M relativistisch ( v ) = m 1 − v 2 c 2 {\displaystyle M_{\text{relativistisch}}(\mathbf {v} )={\frac {m}{\sqrt {1-{\frac {\mathbf {v} ^{2}}{c^{2}}}}}}}
y n + 2 y ( n − 1 ) = e j n Φ m i t j = ( − 1 ) {\displaystyle yn+2y(n-1)=e^{jn\Phi }mitj={\sqrt {(}}-1)}
y n + 2 y ( n − 1 ) = e j n Φ m i t j = − 1 {\displaystyle yn+2y(n-1)=e^{jn\Phi }mitj={\sqrt {-1}}}